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Trabalho de evento
Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations (2015)
Melioli, Claudio; Dal Pino, Elisabete Maria de Gouveia
Source: Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Conference titles: IAU Symposium. Unidade: IAG
Subjects: GALÁXIAS SEY FERT, JATOS (ASTRONOMIA), HIDRODINÂMICA
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ABNT
MELIOLI, Claudio e DAL PINO, Elisabete Maria de Gouveia. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921315002550. Acesso em: 13 nov. 2024.
APA
Melioli, C., & Dal Pino, E. M. de G. (2015). Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations. In Proceedings IAU Symposium, 313: Extragalactic jets from every angle. Paris: International Astronomical Union. doi:10.1017/S1743921315002550
NLM
Melioli C, Dal Pino EM de G. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations [Internet]. Proceedings IAU Symposium, 313: Extragalactic jets from every angle. 2015 ;[citado 2024 nov. 13 ] Available from: https://doi.org/10.1017/S1743921315002550
Vancouver
Melioli C, Dal Pino EM de G. Gas outflow in Seyfert galaxies: 3D radiative cooling hydrodynamical simulations [Internet]. Proceedings IAU Symposium, 313: Extragalactic jets from every angle. 2015 ;[citado 2024 nov. 13 ] Available from: https://doi.org/10.1017/S1743921315002550
Trabalho de evento
An empirical pipeline for determining the viscosity parameter for Be star disks (2015)
Rímulo, Leandro R; Carciofi, Alex Cavaliéri; Rivinius, Thomas; Haubois, Xavier
Source: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Conference titles: IAU Symposium. Unidade: IAG
Subjects: HIDRODINÂMICA, TRANSFERÊNCIA RADIATIVA, FOTOMETRIA, ESTRELAS, PERDA DE MASSA
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
RÍMULO, Leandro R et al. An empirical pipeline for determining the viscosity parameter for Be star disks. 2015, Anais.. Paris: International Astronomical Union, 2015. Disponível em: https://doi.org/10.1017/S1743921314006541. Acesso em: 13 nov. 2024.
APA
Rímulo, L. R., Carciofi, A. C., Rivinius, T., & Haubois, X. (2015). An empirical pipeline for determining the viscosity parameter for Be star disks. In New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. Paris: International Astronomical Union. doi:10.1017/S1743921314006541
NLM
Rímulo LR, Carciofi AC, Rivinius T, Haubois X. An empirical pipeline for determining the viscosity parameter for Be star disks [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. 2015 ;[citado 2024 nov. 13 ] Available from: https://doi.org/10.1017/S1743921314006541
Vancouver
Rímulo LR, Carciofi AC, Rivinius T, Haubois X. An empirical pipeline for determining the viscosity parameter for Be star disks [Internet]. New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry: Proceedings of IAU Symposium, 307. 2015 ;[citado 2024 nov. 13 ] Available from: https://doi.org/10.1017/S1743921314006541
Artigo de periodico
On the controversy regarding the effect of flow shear on the Strouhal number of cylinder vortex shedding (2013)
Gennaro, Elmer Mateus; Colaciti, Alysson Kennerly; Medeiros, Marcello Augusto Faraco de
Source: Aerospace Science and Technology. Unidade: EESC
Subjects: HIDRODINÂMICA, EQUAÇÕES
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ABNT
GENNARO, Elmer Mateus e COLACITI, Alysson Kennerly e MEDEIROS, Marcello Augusto Faraco de. On the controversy regarding the effect of flow shear on the Strouhal number of cylinder vortex shedding. Aerospace Science and Technology, v. 29, n. 1, p. 313-320, 2013Tradução . . Disponível em: https://doi.org/10.1016/j.ast.2013.04.002. Acesso em: 13 nov. 2024.
APA
Gennaro, E. M., Colaciti, A. K., & Medeiros, M. A. F. de. (2013). On the controversy regarding the effect of flow shear on the Strouhal number of cylinder vortex shedding. Aerospace Science and Technology, 29( 1), 313-320. doi:10.1016/j.ast.2013.04.002
NLM
Gennaro EM, Colaciti AK, Medeiros MAF de. On the controversy regarding the effect of flow shear on the Strouhal number of cylinder vortex shedding [Internet]. Aerospace Science and Technology. 2013 ; 29( 1): 313-320.[citado 2024 nov. 13 ] Available from: https://doi.org/10.1016/j.ast.2013.04.002
Vancouver
Gennaro EM, Colaciti AK, Medeiros MAF de. On the controversy regarding the effect of flow shear on the Strouhal number of cylinder vortex shedding [Internet]. Aerospace Science and Technology. 2013 ; 29( 1): 313-320.[citado 2024 nov. 13 ] Available from: https://doi.org/10.1016/j.ast.2013.04.002
Artigo de periodico
SPH simulations of clumps formation by dissipative collision of molecular clouds (2000)
Marinho, E. P.; Lépine, Jacques Raymond Daniel
Source: Astronomy and Astrophysics Supplement Series. Unidade: IAG
Subjects: ASTRONOMIA, RADIOASTRONOMIA, ASTROFÍSICA ESTELAR, HIDRODINÂMICA
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ABNT
MARINHO, E. P. e LÉPINE, Jacques Raymond Daniel. SPH simulations of clumps formation by dissipative collision of molecular clouds. Astronomy and Astrophysics Supplement Series, v. 142, n. 1, p. 165-179, 2000Tradução . . Disponível em: https://doi.org/10.1051/0004-6361:20011352. Acesso em: 13 nov. 2024.
APA
Marinho, E. P., & Lépine, J. R. D. (2000). SPH simulations of clumps formation by dissipative collision of molecular clouds. Astronomy and Astrophysics Supplement Series, 142( 1), 165-179. doi:10.1051/0004-6361:20011352
NLM
Marinho EP, Lépine JRD. SPH simulations of clumps formation by dissipative collision of molecular clouds [Internet]. Astronomy and Astrophysics Supplement Series. 2000 ; 142( 1): 165-179.[citado 2024 nov. 13 ] Available from: https://doi.org/10.1051/0004-6361:20011352
Vancouver
Marinho EP, Lépine JRD. SPH simulations of clumps formation by dissipative collision of molecular clouds [Internet]. Astronomy and Astrophysics Supplement Series. 2000 ; 142( 1): 165-179.[citado 2024 nov. 13 ] Available from: https://doi.org/10.1051/0004-6361:20011352
Artigo de periodico
Study of ferrocholesteric discotic and calamitic lyotropics by optical microscopy and X-ray diffraction (1984)
Figueiredo Neto, A. M. ; Liebert, L.; Levelut, A. M.
Source: Journal de Physique Lettres. Unidade: IF
Subjects: CRISTAIS LÍQUIDOS, FLUÍDOS COMPLEXOS, QUÍMICA COLOIDAL, HIDRODINÂMICA, DIFRAÇÃO POR RAIOS X, MICROSCÓPIO ÓTICO
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
FIGUEIREDO NETO, A. M. e LIEBERT, L. e LEVELUT, A. M. Study of ferrocholesteric discotic and calamitic lyotropics by optical microscopy and X-ray diffraction. Journal de Physique Lettres, v. 45, n. 9, p. 1505-1512, 1984Tradução . . Disponível em: https://doi.org/10.1051/jphys:019840045090150500. Acesso em: 13 nov. 2024.
APA
Figueiredo Neto, A. M., Liebert, L., & Levelut, A. M. (1984). Study of ferrocholesteric discotic and calamitic lyotropics by optical microscopy and X-ray diffraction. Journal de Physique Lettres, 45( 9), 1505-1512. doi:10.1051/jphys:019840045090150500
NLM
Figueiredo Neto AM, Liebert L, Levelut AM. Study of ferrocholesteric discotic and calamitic lyotropics by optical microscopy and X-ray diffraction [Internet]. Journal de Physique Lettres. 1984 ; 45( 9): 1505-1512.[citado 2024 nov. 13 ] Available from: https://doi.org/10.1051/jphys:019840045090150500
Vancouver
Figueiredo Neto AM, Liebert L, Levelut AM. Study of ferrocholesteric discotic and calamitic lyotropics by optical microscopy and X-ray diffraction [Internet]. Journal de Physique Lettres. 1984 ; 45( 9): 1505-1512.[citado 2024 nov. 13 ] Available from: https://doi.org/10.1051/jphys:019840045090150500

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